New Cold Subdwarf Discoveries from Backyard Worlds and a Metallicity Classification System for T Subdwarfs

Abstract We report the results of a spectroscopic survey of candidate T subdwarfs identified by the Backyard Worlds: Planet 9 program. Near-infrared spectra of 31 sources with red J − W2 colors and large J -band reduced proper motions show varying signatures of subsolar metallicity, including strong collision-induced H 2 absorption, obscured methane and water features, and weak K i absorption. These metallicity signatures are supported by spectral model fits and 3D velocities, indicating thick disk and halo population membership for several sources. We identify three new metal-poor T subdwarfs ([M/H] ≲ –0.5), CWISE J062316.19+071505.6, WISEA J152443.14−262001.8, and CWISE J211250.11-052925.2; and 19 new “mild” subdwarfs with modest metal deficiency ([M/H] ≲ −0.25). We also identify three metal-rich brown dwarfs with thick disk kinematics. We provide kinematic evidence that the extreme L subdwarf 2MASS J053253.46+824646.5 and the mild T subdwarf CWISE J113010.07+313944.7 may be part of the Thamnos population, while the T subdwarf CWISE J155349.96+693355.2 may be part of the Helmi stream. We define a metallicity classification system for T dwarfs that adds mild subdwarfs (d/sdT), subdwarfs (sdT), and extreme subdwarfs (esdT) to the existing dwarf sequence. We also define a metallicity spectral index that correlates with metallicities inferred from spectral model fits and iron abundances from stellar primaries of benchmark T dwarf companions. This expansion of the T dwarf classification system supports investigations of ancient, metal-poor brown dwarfs now being uncovered in deep imaging and spectroscopic surveys.

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Publication Details

Journal
The Astrophysical Journal
Published
2025-03-20
DOI
https://doi.org/10.3847/1538-4357/adb39f
Citations
13
Primary Topic
Geological and Geochemical Analysis
Type
article
Field-Weighted Citation Impact
24.26
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article

New Cold Subdwarf Discoveries from Backyard Worlds and a Metallicity Classification System for T Subdwarfs

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13 citations
The Astrophysical Journal
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article

New Cold Subdwarf Discoveries from Backyard Worlds and a Metallicity Classification System for T Subdwarfs

Adam C. Schneider, Jean Marc Gantier, Jacqueline K. Faherty, Paul Beaulieu, Jim Walla, Martin Kabatnik, Dan Caselden, William Pendrill, Adam J. Burgasser, Ken Hinckley, Frank Kiwy, J. Davy Kirkpatrick, Thomas P. Bickle, Jonathan Gagné, Leslie K. Hamlet, Zbigniew Wędracki, Arttu Sainio, Christopher A. Theissen, Hunter Brooks, Austin Rothermich, Chih-Chun Hsu, Michaël Marsset, Nikolaj Stevnbak Andersen, Aaron Meisner, Emma Softich, Melina Thévenot, Léopold Gramaize, Étienne Artigau, Christian Aganze, J. Schümann, Guillaume Colin, Marc J. Kuchner, Preethi R. Karpoor, Roman Gerasimov, David W. Martin, Diego H. Massat
article en
13 citations

Abstract

Abstract We report the results of a spectroscopic survey of candidate T subdwarfs identified by the Backyard Worlds: Planet 9 program. Near-infrared spectra of 31 sources with red J − W2 colors and large J -band reduced proper motions show varying signatures of subsolar metallicity, including strong collision-induced H 2 absorption, obscured methane and water features, and weak K i absorption. These metallicity signatures are supported by spectral model fits and 3D velocities, indicating thick disk and halo population membership for several sources. We identify three new metal-poor T subdwarfs ([M/H] ≲ –0.5), CWISE J062316.19+071505.6, WISEA J152443.14−262001.8, and CWISE J211250.11-052925.2; and 19 new “mild” subdwarfs with modest metal deficiency ([M/H] ≲ −0.25). We also identify three metal-rich brown dwarfs with thick disk kinematics. We provide kinematic evidence that the extreme L subdwarf 2MASS J053253.46+824646.5 and the mild T subdwarf CWISE J113010.07+313944.7 may be part of the Thamnos population, while the T subdwarf CWISE J155349.96+693355.2 may be part of the Helmi stream. We define a metallicity classification system for T dwarfs that adds mild subdwarfs (d/sdT), subdwarfs (sdT), and extreme subdwarfs (esdT) to the existing dwarf sequence. We also define a metallicity spectral index that correlates with metallicities inferred from spectral model fits and iron abundances from stellar primaries of benchmark T dwarf companions. This expansion of the T dwarf classification system supports investigations of ancient, metal-poor brown dwarfs now being uncovered in deep imaging and spectroscopic surveys.

The Astrophysical JournalVol. 982(2)
Openalex Percentile: Top 0%
Geological and Geochemical Analysis
24.26
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